Accession Number : ADA522777


Title :   Constraints on the Dark Matter Particle Mass from the Number of Milky Way Satellites


Descriptive Note : Research rept.


Corporate Author : NAVAL RESEARCH LAB PATUXENT RIVER MD


Personal Author(s) : Polisensky, Emil ; Ricotti, Massimo


Full Text : https://apps.dtic.mil/dtic/tr/fulltext/u2/a522777.pdf


Report Date : 12 Apr 2010


Pagination or Media Count : 16


Abstract : We have conducted N-body simulations of the growth of Milky Way-sized halos in cold and warm dark matter cosmologies. The number of dark matter satellites in our simulated Milky Ways decreases with decreasing mass of the dark matter particle. Assuming that the number of dark matter satellites exceeds or equals the number of observed satellites of the Milky Way we derive lower limits on the dark matter particle mass. We find with 95% confidence ms 11.8 keV for a sterile neutrino produced by the Dodelson & Widrow mechanism and mWDM 2.1 keV for a thermal dark matter particle. The recent discovery of many new dark matter dominated satellites of the Milky Way in the Sloan Digital Sky Survey allows us to set lower limits comparable to constraints from the complementary methods of Lyman- forest modeling and the unresolved cosmic X-ray background. Future surveys like LSST, DES, PanSTARRS, and SkyMapper have the potential to discover many more satellites and further improve constraints on the dark matter particle mass.


Descriptors :   *ARTIFICIAL SATELLITES , SURVEYS , GALAXIES , N BODY PROBLEM , COMPUTERIZED SIMULATION


Subject Categories : Astrophysics
      Celestial Mechanics
      Computer Programming and Software
      Nuclear Physics & Elementary Particle Physics


Distribution Statement : APPROVED FOR PUBLIC RELEASE